2013
DOI: 10.1155/2013/251498
|View full text |Cite
|
Sign up to set email alerts
|

A Study on Some Special Forms of Holographic Ricci Dark Energy in Fractal Universe

Abstract: We have considered the modified and the extended holographic Ricci dark energy models (MHRDE and EHRDE) in fractal universe. We have assumed a time-like fractal profile V = − , where = 4(1 − ). We have reconstructed the Hubble parameter , the energy density, the equations of state parameter , and the deceleration parameter for both MHRDE and EHRDE.

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1
1
1

Citation Types

1
9
0

Year Published

2014
2014
2020
2020

Publication Types

Select...
6

Relationship

0
6

Authors

Journals

citations
Cited by 10 publications
(10 citation statements)
references
References 33 publications
1
9
0
Order By: Relevance
“…In an expanding universe such as the one we have experienced, the scale factor increases monotonically as time passes, hence the redshift parameter has positive values which mean distant galaxies appear redshifted. On the other hand, (i) one can also extend our results by considering fractal description of the extended holographic energy [47], modified holographic Ricci dark energy [48], and new agegraphic dark energy [18], (ii) in Reference [49], the fractal ghost reconstruction of quintessence field was achieved. After comparing our manuscript with this paper, it can be seen that all of our results are agree with and extend those ones obtained in Reference [49].…”
Section: A Then´1supporting
confidence: 58%
“…In an expanding universe such as the one we have experienced, the scale factor increases monotonically as time passes, hence the redshift parameter has positive values which mean distant galaxies appear redshifted. On the other hand, (i) one can also extend our results by considering fractal description of the extended holographic energy [47], modified holographic Ricci dark energy [48], and new agegraphic dark energy [18], (ii) in Reference [49], the fractal ghost reconstruction of quintessence field was achieved. After comparing our manuscript with this paper, it can be seen that all of our results are agree with and extend those ones obtained in Reference [49].…”
Section: A Then´1supporting
confidence: 58%
“…In the theory T 1 with ordinary derivatives, the problem has been considered mainly with exotic dark-energy components, in flat 47,[57][58][59][60][61][62][63] as well as non-flat FLRW. 64,65 In these cases, late-time acceleration is possible, although the theoretical motivation is no more robust than in general relativity.…”
Section: About Cosmologymentioning
confidence: 99%
“…While there are some studies about inflation [18,19] and gravitational-wave propagation [20,21] that constrain or propose possible effects in the cosmic microwave background and in gravitational-wave signals in multifractional spacetimes, the problem of dark energy has received less attention, except in the case with ordinary derivatives. The absence of cosmological vacuum solutions in the theory with ordinary derivatives [16] led some to explore scenarios with more or less exotic dark-energy components [22][23][24][25][26][27][28][29] (see also [30,31] for a thermodynamical approach). However, our point of view is that a sensible theory beyond Einstein should be able to describe cosmic acceleration without introducing dark-energy fields by hand.…”
Section: Introductionmentioning
confidence: 99%